We present results for several nearby, resolved dwarf
galaxies imaged with WFPC2 in the framework of our HST
snapshot survey of nearby dwarf galaxy candidates (Seitzer
et al., paper I in this series). All data presented here
were analyzed with the automated photometry package HSTPHOT
(Dolphin et al., paper IV in this series).

Our closest target is the recently discovered Cassiopeia
dwarf spheroidal (dSph) galaxy (Karachentsev &
Karachentseva 1999, A&A, 341, 355), a new Local Group
member and companion of M31 (Grebel & Guhathakurta 1999,
ApJ, 511, 101). Our WFPC2 snapshot data reveal a pronounced
red horizontal branch in Cas dSph. IC\,5152 is a dwarf
irregular (dIrr) just beyond the Local Group. Our data show
a significant intermediate-age population with a strongly
tilted asymptotic giant branch (AGB), a substantial young
population, and a wide giant branch.

Other nearby galaxies to be discussed include NGC\,1560,
ESO\,471-G006, ESO\,470-G018, and KK\,035. Most of these
galaxies are being resolved into stars for the first time.
We describe their properties in detail and derive distances
for all dwarfs with a well-defined tip of the red giant
branch. Membership of these galaxies in nearby groups is
discussed.

Support for this work was provided by NASA through grant
GO-08192.97A from the Space Telescope Science Institute,
which is operated by the Association of Universities for
Research in Astronomy, Inc., under NASA contract NAS5-26555.
EKG acknowledges support by NASA through grant
HF-01108.01-98A from the Space Telescope Science Institute.
EKG and IDK are supported by the Henri Chrétien
International Research Grant administered by the American
Astronomical Society. PG is an Alfred P.\ Sloan Research
Fellow.